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S. Sulis

33 papers hereh-index 10389 citations44 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author8
  • middle author22
  • last author1

Across the 31 of 33 papers where every author was matched, so the position is known.

fields
  • astro-ph.EP23
  • astro-ph.SR5
  • astro-ph.IM2
  • stat.AP2
  • math.ST1
same name
  • S. Sulis — 25 papers, h 5
  • S. Sulis — 9 papers, h 30
  • S. Sulis — 5 papers, h 3
  • S. Sulis — 3 papers
  • S. Sulis — 1 paper, h 2
  • S. Sulis — 1 paper, h 1

Either other researchers who publish under this name, or the same person where the external sources have not merged their records.

identity via Semantic Scholar / OpenAlex

activity
20162026
most citedTransit detection of the long-period volatile-rich super-Earth ν2 Lupi d with CHEOPS

87 citations · 502 across the 31 of their papers we have counts for

collaborators
Showing 2020Show all

3 papers · 1 filter

astro-ph.IM2020

Some detection tests for low complexity data models and unknown background distribution

D. Mary, S. Bourguignon, E. Roquain +2

We consider several detection situations where, under the alternative hypothesis, the signal admits a low complexity model and, under both the null and the alternative hypotheses,…

astro-ph.EP2020★ 31 cited

Mitigating flicker noise in high-precision photometry. I -- Characterization of the noise structure, impact on the inferred transit parameters, and predictions for CHEOPS observations

S. Sulis, M. Lendl, S. Hofmeister +4

In photometry, the short-timescale stellar variability ("flicker"), such as that caused by granulation and oscillations, can reach amplitudes comparable to the transit depth of Ear…

astro-ph.EP2020★ 20 cited

3D magneto-hydrodynamical simulations of stellar convective noise for improved exoplanet detection. I. Case of regularly sampled radial velocity observations

S. Sulis, D. Mary, L. Bigot

Convective motions at the stellar surface generate a stochastic colored noise source in the radial velocity (RV) data. This noise impedes the detection of small exoplanets. Moreove…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.